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Signatures of Confined and Eruptive Solar Flares in Microwave Spectra

We describe how microwave spectra of confined flares differ from those of eruptive flares. All 29 confined ≥M1.4 soft X-ray flares from NOAA Active Region 12192 in 2014 October that were observed by the Radio Solar Telescope Network in the >300 MHz microwave range (encompassing RSTN frequencies from...

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Auteurs principaux: E. W. Cliver, M. Kazachenko, H. S. Hudson, T. Alberti, M. Laurenza, S. M. White, P. T. Gallagher
Format: Artigo
Langue:Inglês
Publié: IOP Publishing 2025-01-01
Collection:The Astrophysical Journal
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Accès en ligne:https://doi.org/10.3847/1538-4357/adfbe5
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